Challenges in coronagraph optical design

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Citation (Scopus)

Abstract

The point spread function (PSF) for astronomical telescopes and instruments depends not only on geometric aberrations and scalar wave diffraction, but also on the apodization and wavefront errors introduced by coatings on reflecting and transmitting surfaces within the optical system. Geometrical ray tracing provides incomplete image simulations for exoplanet coronagraphs with the goal of resolving planets with a brightness less than 10^-9 of their star located within 3 Airy disk radii. The Polaris-M polarization analysis program calculates uncorrected coating polarization aberrations couple around 10^-5 light into crossed polarized diffraction patterns about twice Airy disk size. These wavefronts not corrected by the deformable optics systems. Polarization aberrations expansions have shown how image defects scale with mirror coatings, fold mirror angles, and numerical aperture.

Original languageEnglish (US)
Title of host publicationOptical Modeling and Performance Predictions IX
PublisherSPIE
Volume10374
ISBN (Electronic)9781510612051
DOIs
StatePublished - Jan 1 2017
EventOptical Modeling and Performance Predictions IX 2017 - San Diego, United States
Duration: Aug 7 2017Aug 8 2017

Other

OtherOptical Modeling and Performance Predictions IX 2017
CountryUnited States
CitySan Diego
Period8/7/178/8/17

Fingerprint

Coronagraph
Optical design
coronagraphs
Optical Design
Aberrations
Aberration
Coating
aberration
Polarization
Wavefronts
coatings
Wave Front
Coatings
Mirror
Mirrors
polarization
Astronomical Telescopes
mirrors
Image Simulation
Wave Diffraction

Keywords

  • Coronagraph
  • Imaging
  • Polarization
  • Polarization aberration
  • Polarization ray tracing

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

Cite this

Chipman, R. A. (2017). Challenges in coronagraph optical design. In Optical Modeling and Performance Predictions IX (Vol. 10374). [1037403] SPIE. https://doi.org/10.1117/12.2274055

Challenges in coronagraph optical design. / Chipman, Russell A.

Optical Modeling and Performance Predictions IX. Vol. 10374 SPIE, 2017. 1037403.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Chipman, RA 2017, Challenges in coronagraph optical design. in Optical Modeling and Performance Predictions IX. vol. 10374, 1037403, SPIE, Optical Modeling and Performance Predictions IX 2017, San Diego, United States, 8/7/17. https://doi.org/10.1117/12.2274055
Chipman RA. Challenges in coronagraph optical design. In Optical Modeling and Performance Predictions IX. Vol. 10374. SPIE. 2017. 1037403 https://doi.org/10.1117/12.2274055
Chipman, Russell A. / Challenges in coronagraph optical design. Optical Modeling and Performance Predictions IX. Vol. 10374 SPIE, 2017.
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